X-ray line signal from decaying axino warm dark matter

作者:Choi Ki Young*; Seto Osamu
来源:Physics Letters B, 2014, 735: 92-94.
DOI:10.1016/j.physletb.2014.06.008

摘要

We consider axino warm dark matter in a supersymmetric axion model with R-parity violation. In this scenario, axino with the mass m (a) over tilde similar or equal to 7 keV can decay into photon and neutrino resulting in the X-ray line signal at 3.5 keV, which might be the origin of unidentified X-ray emissions from galaxy clusters and Andromeda galaxy detected by the XMM-Newton X-ray observatory.

  • 出版日期2014-7-30